Haehnelt Martin G
Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK.
Philos Trans A Math Phys Eng Sci. 2005 Mar 15;363(1828):705-13; discussion 713. doi: 10.1098/rsta.2004.1522.
Massive black holes appear to be an essential ingredient of massive galactic bulges but little is known yet to what extent massive black holes reside in dwarf galaxies and globular clusters. Massive black holes most likely grow by a mixture of merging and accretion of gas in their hierarchically merging host galaxies. While the hierarchical merging of dark matter structures extends to sub-galactic scales and very high redshift, it is uncertain if the same is true for the build-up of massive black holes. I discuss here some of the relevant problems and open questions.
超大质量黑洞似乎是大型星系核球的重要组成部分,但目前对于超大质量黑洞在矮星系和球状星团中的存在程度知之甚少。超大质量黑洞很可能是通过在其分层合并的宿主星系中合并和吸积气体的混合过程而增长的。虽然暗物质结构的分层合并延伸到次星系尺度和非常高的红移,但超大质量黑洞的形成是否也是如此尚不确定。我在此讨论一些相关问题和未解决的疑问。